A dark matter model that reconciles tensions between the cosmic-ray e ± excess and the gamma-ray and CMB constraints-Reference-Cited by-同舟云学术

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A dark matter model that reconciles tensions between the cosmic-ray e ± excess and the gamma-ray and CMB constraints

Published:2017-10 Issue: Volume:773 Page:448-454
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Xiang Qian-Fei,Bi Xiao-Jun,Lin Su-Jie,Yin Peng-Fei

Funder

National Key Program for Research and Development

National Natural Science Foundation of China

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference59 articles.

1. Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation;Komatsu;Astrophys. J. Suppl.,2009

2. Planck 2015 results. XIII. Cosmological parameters;Ade;Astron. Astrophys.,2016

3. First result from the Alpha Magnetic Spectrometer on the International Space Station: precision measurement of the positron fraction in primary cosmic rays of 0.5–50 GeV;Aguilar;Phys. Rev. Lett.,2013

4. Pulsars as the sources of high energy cosmic ray positrons;Hooper;J. Cosmol. Astropart. Phys.,2009

5. TeV gamma rays from Geminga and the origin of the GeV positron excess;Yuksel;Phys. Rev. Lett.,2009

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3. Proposition of FSR Photon Suppression Employing a Two-Positron Decay Dark Matter Model to Explain Positron Anomaly in Cosmic Rays;Universe;2023-08-15

4. Confronting cosmic ray electron and positron excesses with hybrid triplet Higgs portal dark matter *;Chinese Physics C;2022-06-01

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